J/A+A/597/A51ivo://CDS.VizieR/J/A+A/597/A51doi:10.26093/cds/vizier.35970051CDSVika M.Ciesla L.Charmandaris V. Xilouris E.M.Lebouteiller V.2017-10-09T13:34:47Z2016-12-21T09:21:57ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxiescatalogsphotometryWe provide the basic integrated physical properties of all the galaxies contained in the full Cornell Atlas of Spitzer/IRS Sources (CASSIS) with available broad-band photometry from UV to 22 microns. We have collected broad-band photometric measurements in 14 wavelengths from available public surveys in order to study the spectral energy distribution (SED) of each galaxy in CASSIS, thus constructing a final sample of 1146 galaxies in the redshift range 0<z<2.5. The SEDs are modelled with the CIGALE code which relies on the energy balance between the absorbed stellar and the dust emission while taking into account the possible contribution due to the presence of an active galactic nucleus (AGN). We split the galaxies in three groups, a low-redshift (z<0.1), a mid-redshift (0.1=<z<0.5) and a high-redshift (z>=0.5) sub-sample and find that the vast majority of the Spitzer/IRS galaxies are star-forming and lie on or above the star-forming main sequence of the corresponding redshift. Moreover, the emission of Spitzer/IRS galaxies with z<0.1 is mostly dominated by star-formation, galaxies in the mid-redshift bin are a mixture of star forming and AGN galaxies, while half of the galaxies with z>=0.5 show moderate or high AGN activity. Additionally, using rest-frame NUV-r colour, Sersic indices, optical [OIII] and [NII] emission lines we explore the nature of these galaxies by investigating further their structure as well as their star-formation and AGN activity. Using a colour magnitude diagram we confirm that 97% of the galaxies with redshift smaller than 0.5 have experienced a recent star-formation episode. For a sub-sample of galaxies with available structural information and redshift smaller than 0.3 we find that early-type galaxies are placed below the main sequence, while late-type galaxies are found on the main- sequence as expected. Finally, for all the galaxies with redshift smaller than 0.5 and available optical spectral line measurements we compare the ability of CIGALE to detect the presence of an AGN in contrast to the optical spectra classification. We find that galaxies with high AGN luminosity, as calculated by CIGALE, are most likely to be classified as composite or AGNs by optical spectral lines.2017A&A...597A..51Vhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/597/A51CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/597/A51https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/597/A51http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/597/A51https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/597/A51https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/597/A51http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/597/A51GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/597/A51/cassis (IDs, physical parameters for 1146 of the CASSIS sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/597/A51/cassis?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/597/A51/cassis?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/597/A51/cassis?GETtext/xml+votable180.050000true0.7040.7510.0055555555555555565/1519 1828 2286 2335 2361 2410 2538 4422 6/286 579 687 697 747 1008 2052 2245 2248 2564 4121 4215 4285 4290 4303 4369 4405 4412 4447 4469 4506 4536 4545 4649 4835 4839 4867 4898 4992-4993 5016 5033 5037 5039 5090 5176 5200 5213 5221 5244 5257 5284 5290 5333 5356 5359 5395 5437 5439 5464 5481 5495 5500 5552 5556 5568 5576 5597 5604 5607 5687 5711-5712 5730 5738 5741 5744 5746 5752-5754 5765 5767 5773 5776 5793 5810 5814 5817 5819 5839 5865 5926 5931-5932 5950 5970 5998 6005 6009 6028 6057 6070-6071 6073 6075 6104 6109 6112 6114-6115 6120-6121 6127 6212 6262 6293 6348 6419 6446 6449 6499 6508 6515 6518 6532 6535-6536 6539 6544 6555 6609 6623 7178 7182 7208 7229 7243 7259 7261 7266 7269 7271 7277 7284 7298 7300-7301 7303-7304 7308-7310 7318-7321 7364-7365 7386 7424-7425 7429 7443 7446 7456 7460 7466 7477 7484 7502 7522 7552 7570 7741 7763 7777 7896 7954 8017 8133 8208-8209 8214 8216-8217 8225 8230 8233 8235 8268-8269 8299 8322 8509 8528 8555 8557 8590 8626-8627 8636-8637 8675 8695 8791 8881 8893 8906 8922 8926-8927 8941 8943 9018-9019 9070 9072 9085 9098 9135 9148 9150-9151 9166 9170 9181-9182 9190 9194 9196 9205 9209-9211 9223 9231 9246 9252 9262 9328 9397 9402 9417 9453-9455 9459 9461 9469 9471 9483 9504-9505 9510 9513 9516 9519 9610 9612 9617 9632 9634-9635 9639 9645 9740-9741 9743 9754 9763 9766 9770 9793-9794 9796-9797 9799 9802 9807 9809 9814 9819-9820 9822 9829 9836 9841 9856 9879 9924 9943 9959 9974-9975 9978 10022 10039 10061 10072 10075 10086 10096-10097 10104 10121 10123 10144 10146-10147 10150 10156 10182-10183 10187 10189-10191 10200 10212-10214 10217 10269 10281 10321 10324 10355 10378-10379 10394 10399 10422 10432 10440 10442 10472 10501 10512-10513 10515-10518 10561 10578 10588 10599 10628 10641 10669-10671 10691 10694 10709 10716 10761 10881 10912 10925 11009-11010 11071 11101 11125 11127 11132 11217 11258-11259 11264 11283 11326 11353 11356 11380-11382 11386 11388-11389 11406 11445 11457 11461-11462 11472 11481 11488 11491 11497 11500 11502 11504 11521 11524 11585 11590 11783 11786-11790 11800 11808 11884 11908 11930-11931 11943 12047 12317 12402 12409 12630-12632 12892 13380 13488 13496 13601 16011 16478 16500 16509 16652 16690 16712 16882 17203 17214 17245 17252 17264 17306 17492 17506 17564 17582 17606 17614 17677 17683 17686 17692 17694 17712-17713 17716 17761 17795 17812 17816 17819 17850 17866 17868 17905 17979 18009-18010 18012 18017 18019 18024 18028 18034 18038 18074 18086 18092 18127 18207 18302 18367 18387 18519 18524 18601 18607 18749 18757 18767 18793-18794 18796 18864 18895 18897 18919 19026 19033 19053 19099 19139 19216 19283 19296 19315 19398 19416 19419 19433 19457 19617 19619 19637 19661 19688 19700 19730 19735 19738 19741-19742 19746 19762 19767 19797 19804 19830 19846 19932 19934 19959 19966 20061 20099 20118 20137 20208 20211 20290 20379 20389 21847 21996 22007 23059-23060 23073 23078 23182 23194 23198 23210-23211 23233 24829 25094 25216 25245 25582 25595 25742 25851 25916 25919 25936 25974 25977 25982 25986 26000 26002 26019 26035 26041 26064 26066 26070-26071 26087 26096 26100 26142 26161 26173 26178 26183-26184 26225 26230 26260 26267 26292 26310 26323 26393 26407 26491 26509 26540 26572 26593 26932 26984 26989 26996 27005 27023 27067 27081 27085 27105 27114 27225 27227 27230 27256 27258-27259 27295 27342-27343 27349 27362 27428 27480 27483 27502 27514 27606 27720 27734 27767 27771 27848 27955 27976 28074-28075 28083 28113 28152 28164 28172 28188 28350 28376 28471 28492 28517 28522 28532 28540 28591 28609 30040 31327 31339 31401 31422 31442 31650-31651 31729 32362 32408 32422 32548 33204 33409 34020 34652 34739 35383 35388 35390 35473 35582 35774 35872 35935 36352 36559 36723 36733 36763 36766-36767 36771 36781-36783 36785-36786 44988 45044 45564 45763 46566 46568 47007 47375 47957 48478 48561 48652 48865 49094https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/597/A51?format=asciiOpticaldefaultJ/A+A/597/A51/cassisIDs, physical parameters for 1146 of the CASSIS sampleA[0/4] Classification (1)meta.codeintB[0/3] Classification (2)meta.codeintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAORkeySpitzer/IRS identification keymeta.idintRAJ2000Right ascension of the Spitzer/IRS source (J2000)degpos.eq.ra;meta.mainDEJ2000Declination of the Spitzer/IRS source (J2000)degpos.eq.dec;meta.mainzRedshift from NEDsrc.redshiftfloatM*Stellar mass as measured by CIGALEsolMassphys.massdoublee_M*Uncertainty of stellar mass as measured by CIGALEsolMassstat.errordoubleSFRStar-formation rate as measured by CIGALEsolMass/yrphys.SFRdoublee_SFRUncertainty of star- formation rate as measured by CIGALEsolMass/yrstat.error;phys.SFRdoubleAgeStellar age as measured by CIGALEMyrtime.ageinte_AgeUncertainty of stellar age as measured by CIGALEMyrstat.error;time.ageintAE(B-V)Attenuation of young stellar populations as measured by CIGALEphys.absorptionfloate_AE(B-V)Uncertainty of E(B-V) attenuation of young stellar populations as measured by CIGALEstat.errorfloatfAGNContribution of an AGN to the total IR luminosity as measured by CIGALEphys.luminosity;arith.ratiofloate_fAGNUncertainty of contribution of an AGN to the total IR luminosity as measured by CIGALEstat.errorfloatLAGNAGN luminosity as measured by CIGALEWphys.luminositydoublee_LAGNUncertainty of AGN luminosity as measured by CIGALEWstat.errordoubleLdustDust luminosity as measured by CIGALEWphys.luminositydoublee_LdustUncertainty of dust luminosity as measured by CIGALEWstat.errordoubleAFUVThe attenuation in the FUV as measured by CIGALEmagphys.absorptionfloatchi2rMinimised chi square of the fitstat.fit.chi2floatNEDnameGalaxy name from NEDmeta.idcharf[0/1] Flag where 1 indicates saturation flag in SDSS datameta.codeintNEDSimbad column added by the CDSmeta.ref.urlchar